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  Dense gas in the Galactic central molecular zone is warm and heated by turbulence

Ginsburg, A., Henkel, C., Ao, Y., Riquelme, D., Kauffmann, J., Pillai, T., et al. (2016). Dense gas in the Galactic central molecular zone is warm and heated by turbulence. Astronomy & Astrophysics, 586: A50, pp. 1-31. doi:10.1051/0004-6361/201526100.

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 Creators:
Ginsburg, Adam, Author
Henkel, Christian, Author
Ao, Yiping, Author
Riquelme, Denise, Author
Kauffmann, Jens, Author
Pillai, Thushara, Author
Mills, Elisabeth A. C., Author
Requena-Torres, Miguel A., Author
Immer, Katharina, Author
Testi, Leonardo, Author
Ott, Juergen, Author
Bally, John, Author
Battersby, Cara, Author
Darling, Jeremy, Author
Aalto, Susanne, Author
Stanke, Thomas, Author
Kendrew, Sarah, Author
Kruijssen, J. M. Diederik1, Author           
Longmore, Steven, Author
Dale, James, Author
Guesten, Rolf, AuthorMenten, Karl M., Author more..
Affiliations:
1Computational Structure Formation, MPI for Astrophysics, Max Planck Society, ou_2205642              

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Language(s): eng - English
 Dates: 2016-02
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/201526100
Other: LOCALID: 2262997
 Degree: -

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Title: Astronomy & Astrophysics
  Abbreviation : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 586 Sequence Number: A50 Start / End Page: 1 - 31 Identifier: ISSN: 0004-6361